Results 211 to 220 of about 104,360 (261)

Astrochemical Significance of C₂H₇NO Isomers: A Computational Perspective on Their Stability and Detectability. [PDF]

J Phys Chem A
Noriega L, Gonzalez-Ortiz LA, Ortíz-Chi F, Merino G.   +3 more
europepmc   +1 more source

Generation and UV-photolysis of <i>N</i>-methyleneformamide. [PDF]

Chem Sci
Paczelt V, Drabkin VD, Kühn D, Eckhardt AK.   +3 more
europepmc   +1 more source

Comprehensive Atomistic Simulations of Fischer-Tropsch in Outer Space: Astrocatalysis by Fe₁₃-Supported Nanoclusters on SiO₂. [PDF]

J Phys Chem C Nanomater Interfaces
Pareras G, Cabedo V, McCoustra M, Rimola A.   +3 more
europepmc   +1 more source

Flux equipartition in astrophysical plasma turbulence. [PDF]

Sci Adv
Marino R, Xie JH.
europepmc   +1 more source

Electron-Impact Resonances of Anthracene in the Presence of Methanol: Does the Solvent Identity Matter? [PDF]

J Phys Chem Lett
Lietard A, Verlet JRR.
europepmc   +1 more source

Evidence of the Amino Acids Tyrosine and Phenylalanine in the Interstellar Material of IC348 in Perseus. [PDF]

Life (Basel)
Iglesias-Groth S, Marín Dobrincic M, Pérez Garrido A, Gutierrez C.   +3 more
europepmc   +1 more source

Energy partitioning in H₂ formation on interstellar carbonaceous grains. Insights from <i>ab initio</i> molecular dynamics simulations.

Phys Chem Chem Phys
Jubert L, Martínez-Bachs B, Pareras G, Rimola A.   +3 more
europepmc   +1 more source

X-ray absorption spectroscopy of FeH⁺ to aid its identification in astrochemical environments.

Chem Commun (Camb)
Jin S, Flach M, Ebenbichler A, Cunningham EM, Zamudio-Bayer V, Hirsch K, van der Linde C, Przybilla N, Ončák M, Lau JT, Beyer MK.   +10 more
europepmc   +1 more source

Predicting accurate binding energies and vibrational spectroscopic features of interstellar icy species. A quantum mechanical study.

Phys Chem Chem Phys
Bulik A, Martínez-Bachs B, Bancone N, Mates-Torres E, Corno M, Ugliengo P, Rimola A.   +6 more
europepmc   +1 more source

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The Cool Interstellar Medium

Space Science Reviews, 2005
Infrared spectroscopy and photometry with ISO covering most of the emission range of the interstellar medium has led to important progress in the understanding of the physics and chemistry of the gas, the nature and evolution of the dust grains and also the coupling between the gas and the grains.
Abergel, A., Verstraete, L., Joblin, C., Laureijs, R., A. Miville-Deschênes, M.   +4 more
openaire   +3 more sources